IRAC Monitoring of NGC 4051 for Interday Variability

Details IRAC Monitoring of NGC 4051 for Interday Variability IRAC Monitoring of NGC 4051 for Interday Variability

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop..484g&link_type=abstract

Spitzer Proposal ID #484

Physics

Scientific paper

We will be observing the Seyfert 1.5 NGC 4051 on a daily basis for
approximately 10 days for signs of variability at 3.6 and 5.8 microns.
NGC 4051 has previously shown variability on this timescale at 2.2
microns. Based on the difference in variability at 3.6 and 5.8 microns
limits can be placed on the dust distribution at the nucleus of the AGN.

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